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相关论文: Effects of the interaction between dark energy and…

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We examine different phenomenological interaction models for Dark Energy and Dark Matter by performing statistical joint analysis with observational data arising from the 182 Gold type Ia supernova samples, the shift parameter of the Cosmic…

天体物理学 · 物理学 2009-06-23 Chang Feng , Bin Wang , Elcio Abdalla , Ru-Keng Su

We study a cosmological model in which phantom dark energy is coupled to dark matter by phenomenologically introducing a coupled term to the equations of motion of dark energy and dark matter. This term is parameterized by a dimensionless…

高能物理 - 理论 · 物理学 2009-11-10 Rong-Gen Cai , Anzhong Wang

The cosmological model with an interaction between dynamical quintessence dark energy and cold dark matter is considered. Evolution of a dark energy equation of state parameter is defined by a dark energy adiabatic sound speed and a dark…

宇宙学与河外天体物理 · 物理学 2023-11-08 Roman Neomenko

In the proposed model with interaction between dark energy and dark matter, we consider cosmological scenarios with different equations of state ($w_d$) for dark energy. For both constant and variable equation of state, we analyze solutions…

广义相对论与量子宇宙学 · 物理学 2017-10-18 Supriya Pan , German S. Sharov

We have re-investigated Cosmology involving interaction between Dark matter and Dark Energy in the light of a new parametrization. The new parametrization is based on the hypothesis that when Dark matter and Dark Energy will interact, Dark…

宇宙学与河外天体物理 · 物理学 2023-09-20 Arkajit Aich

Models where Dark Matter and Dark Energy interact with each other have been proposed to solve the coincidence problem. We review the motivations underlying the need to introduce such interaction, its influence on the background dynamics and…

宇宙学与河外天体物理 · 物理学 2016-08-24 B. Wang , E. Abdalla , F. Atrio-Barandela , D. Pavon

We use the latest compilation of observational Hubble parameter measurements estimated with the differential evolution of cosmic chronometers, in combination with the local value of the Hubble constant recently measured with 2.4% precision,…

宇宙学与河外天体物理 · 物理学 2016-07-13 Rafael C. Nunes , Supriya Pan , Emmanuel N. Saridakis

The interacting and holographic dark energy models involve two important quantities. One is the characteristic size of the holographic bound and the other is the coupling term of the interaction between dark energy and dark matter. Rather…

高能物理 - 理论 · 物理学 2008-11-26 Bo Hu , Yi Ling

In this paper, we test the dark matter-dark energy interacting cosmological model with a dynamic equation of state $w_{DE}(z)=w_{0}+w_{1}z/(1+z)$, using type Ia supernovae (SNe Ia), Hubble parameter data, baryonic acoustic oscillation (BAO)…

宇宙学与河外天体物理 · 物理学 2015-04-16 J. S. Wang , F. Y. Wang

In this paper, we have studied an interacting dark energy model. We have assumed the gravitational interaction between the matter fields i.e. between barotropic fluid and the dark energy. The dark energy evolution within the framework of…

广义相对论与量子宇宙学 · 物理学 2023-04-03 Keshav Ram Mishra , Shibesh Kumar Jas Pacif , Rajesh Kumar , Kazuharu Bamba

We investigate phenomenological interactions between dark matter and dark energy and constrain these models by employing the most recent cosmological data including the cosmic microwave background radiation anisotropies from Planck 2015,…

宇宙学与河外天体物理 · 物理学 2017-01-25 André A. Costa , Xiao-Dong Xu , Bin Wang , E. Abdalla

The coupling between the dark components provides a new approach to mitigate the coincidence problem of cosmological standard model. In this paper, dark energy is treated as a fluid with a constant equation of state, whose coupling with…

宇宙学与河外天体物理 · 物理学 2014-08-18 Weiqiang Yang , Lixin Xu

In order to test the possible interaction between dark energy and dark matter, we investigate observational constraints on a phenomenological scenario, in which the ratio between the dark energy and matter densities is proportional to the…

宇宙学与河外天体物理 · 物理学 2015-05-20 Shuo Cao , Nan Liang , Zong-Hong Zhu

Unless some unknown symmetry in Nature prevents or suppresses a non-minimal coupling in the dark sector, the dark energy field may interact with the pressureless component of dark matter. In this paper, we investigate some cosmological…

宇宙学与河外天体物理 · 物理学 2010-04-28 F. E. M. Costa , E. M. Barboza , J. S. Alcaniz

We investigate the dynamical behaviour of a general class of interacting models in the dark sector in which the phenomenological coupling between cold dark matter and dark energy is a power law of the cosmic scale factor. From numerical…

宇宙学与河外天体物理 · 物理学 2017-09-04 F. E. M. Costa , A. O. Ribeiro , F. Roig

The paper deals with a theoretical model for interacting dark energy. The interaction between the cold dark matter (dust) and the dark energy has been assumed to be non-gravitational in nature. Exact analytic cosmological solutions are…

广义相对论与量子宇宙学 · 物理学 2015-07-31 Supriya Pan , Subhra Bhattacharya , Subenoy Chakraborty

Interacting dark energy models may play a crucial role in explaining several important observational issues in modern cosmology and also may provide a solution to current cosmological tensions. Since the phenomenology of the dark sector…

宇宙学与河外天体物理 · 物理学 2023-12-06 Weiqiang Yang , Supriya Pan , Olga Mena , Eleonora Di Valentino

Interactions within the cosmic medium modify its equation of state. We discuss implications of interacting dark energy models both for the spatially homogenous background and for the perturbation dynamics.

广义相对论与量子宇宙学 · 物理学 2009-11-11 Winfried Zimdahl

The interaction between dark matter and dark energy can be incorporated into field theory models of dark energy that have proved successful in alleviating the coincidence problem. We review recent advances in this field, including new…

宇宙学与河外天体物理 · 物理学 2024-02-02 B Wang , E Abdalla , F Atrio-Barandela , D Pavón

Using the data coming from the new 182 Gold type Ia supernova samples, the shift parameter of the Cosmic Microwave Background given by the three-year Wilkinson Microwave Anisotropy Probe observations, and the baryon acoustic oscillation…

天体物理学 · 物理学 2009-06-23 Chang Feng , Bin Wang , Yungui Gong , Ru-Keng Su
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